[en] For the measurement of neutron capture cross sections of noble gases a new experimental technique was developed using high pressure gas targets. By this technique, measurements on five krypton samples with different isotopic composition were performed by which the capture and the total cross sections between 5 and 200 keV were determined in the same experiment with good statistical accuracy. Values of Maxwellian averaged capture cross sections at 30 keV could be derived for the stable isotopes of krypton, as they are required for a quantitative understanding of the s-process of nucleosynthesis. From the systematics of this s-process it was possible to determine the original abundance of krypton in the solar system. The branching of the s-process at Se-79 allowed to determine the temperature of the s-process. A value of kT = 35 keV is adopted by this calculation. (orig.) 891 KBE/orig. 892 HIS